Omega Centauri

Ang Omega Centauri (ω Cen, NGC 5139, Caldwell 80, o Melotte 118) ay isang pabilog na kumpol ng bituin sa konstelasyon ng Centaurus na natuklasan ni Edmond Hall

Omega Centauri
Omega Centauri, isang pabilog na kumpol ng bituin.

Ang Omega Centauri (ω Cen, NGC 5139, Caldwell 80, o Melotte 118) ay isang pabilog na kumpol ng bituin sa konstelasyon ng Centaurus na natuklasan ni Edmond Halley noong 1677.[1] Ito ay matatagpuan sa layong 15,800 taong-liwanag (4,850 parsecs).[2][3]

Ito ang pinakamalaking kilalang pabilog na kumpol ng bituin sa Ariwanas na may diyametrong humigit-kumulang nasa 150 taong-liwanag.[4][5] Tinatayang naglalaman ito ng humigit-kumulang nasa 10 milyong bituin at may 4 milyong masa ng araw.[1][6][7]

May mga ipinapakita ng ebidensya na may isang bihirang itim na butas na may katamtamang masa (intermediate-mass black hole) sa gitna nito, kasama ang mas maliliit na itim na butas na kasinlaki ng bituin (stellar-mass black hole), at natukoy ito sa pamamagitan ng astrometriya.[8][9][10][11][12]

Tingnan din

Mga sanggunian

  1. 1.0 1.1 "Omega Centauri - NASA Science" (sa wikang Ingles). Nakuha noong 2026-08-12.
  2. "eSky: Omega Centauri". www.glyphweb.com. Nakuha noong 2026-08-12.
  3. Berman, Bob (2015-04-24). "Weird Object: Omega Centauri | Astronomy.com". Astronomy Magazine (sa wikang Ingles). Nakuha noong 2026-08-12.
  4. McClure, Bruce (2026-05-06). "Meet Omega Centauri, a giant globular star cluster". EarthSky (sa wikang Ingles). Nakuha noong 2026-08-12.
  5. "Omega Centauri - The glittering giant of the southern skies". ESO (sa wikang Ingles). Nakuha noong 2026-08-12.
  6. "APOD: 2010 March 31 - Millions of Stars in Omega Centauri". apod.nasa.gov. Inarkibo mula sa orihinal noong 2010-04-02. Nakuha noong 2026-08-12.
  7. "Omega Centauri". AAPOD2.COM (sa wikang Ingles). Nakuha noong 2026-08-12.
  8. "Hubble finds evidence for rare black hole in Omega Centauri". ESA (sa wikang Ingles). 2024-10-07. Nakuha noong 2026-08-12.
  9. "Black hole found in Omega Centauri". ESA (sa wikang Ingles). 2008-02-04. Nakuha noong 2026-08-12.
  10. Noyola, E.; Gebhardt, K.; Bergmann, M. (2008). "Gemini and Hubble Space Telescope Evidence for an Intermediate-Mass Black Hole in ω Centauri". The Astrophysical Journal. 676 (2): 1008–1015. arXiv:0801.2782. Bibcode:2008ApJ...676.1008N. doi:10.1086/529002. S2CID 208867075.
  11. Cooper, Keith (2026-07-14). "The 1st of 10,000 'missing' black holes in the Omega Centauri star cluster has been found by the Hubble and James Webb space telescopes". Space.com (sa wikang Ingles). Nakuha noong 2026-08-12.
  12. Häberle, Maximiliam; atbp. (2024-07-10). "Fast-moving stars around an intermediate-mass black hole in ω Centauri". Nature. 631: 285–288. arXiv:2405.06015. Bibcode:2024Natur.631..285H. doi:10.1038/s41586-024-07511-z.

Astronomiya Ang lathalaing ito na tungkol sa Astronomiya ay isang usbong. Makatutulong ka sa Wikipedia sa pagpapalawig nito.

Content Disclaimer

Informasi ini disarikan dari Wikipedia dan disajikan kembali untuk tujuan edukasi. Konten tersedia di bawah lisensi CC BY-SA 3.0. Kami tidak bertanggung jawab atas ketidakakuratan data yang bersumber dari kontribusi publik tersebut.

  1. The information displayed on this website is sourced in part or in whole from Wikipedia and has been adapted for the purpose of restating it. We strive to provide accurate and relevant information, however:
  2. There is no guarantee of absolute accuracy. Wikipedia is an open, collaborative project that can be edited by anyone, so information is subject to change.
  3. It is not intended to constitute professional advice. The content displayed is for informational and educational purposes only. For important decisions (e.g., medical, legal, or financial), please consult a professional.
  4. Content copyright. Wikipedia is licensed under the Creative Commons Attribution-ShareAlike License (CC BY-SA). This means that content may be reused with appropriate attribution and shared under a similar license.
  5. Responsible use. Any risk arising from the use of information from this website is entirely the responsibility of the user.